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Welcome to the ROTSE collaboration.
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The primary goal of the ROTSE project is to achieve
observations in optical light of the massive deep-space
explosions called Gamma-Ray Bursts. To
carry out our program, the small but powerful ROTSE telescopes
are being installed at sites around the world. Here in these
web pages you can learn more about the science, the
operations, and the technology behind ROTSE. |
View a movie of a ROTSE telescope, slewing at top speed.
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From here you can:
- Learn more about the project
- Give feedback or ask questions here
- What are the ROTSE telescopes like?
- Eavesdrop on our real-time operation
- Learn about ROTSE science
- ROTSE-III responses to GRB alerts
- Learn about recent ROTSE transients
- ROTSE Supernova Verification Project (RSVP)
- Access the ROTSE project status
site (collaborators only)
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| A recent image: |
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| Here is an early picture of M31 (the Andromeda
Galaxy), taken by ROTSE-IIIb on Feb 2, 2003, on the third night of
operation.
Here is Comet
C/2001 Q4 (NEAT), as imaged by ROTSE-IIId in Turkey!
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| The ROTSE project is made possible by
grants from NASA, NSF, and the Australian Research Council, and through
participation and support from the University of Michigan, Los Alamos
National Laboratory, and the University of New South Wales.
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